J VI Himalia - Narrowband spectrophotometric support of a C-class asteroid origin

Details J VI Himalia - Narrowband spectrophotometric support of a C-class asteroid origin J VI Himalia - Narrowband spectrophotometric support of a C-class asteroid origin

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..659j&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 659.

Mathematics

Logic

Spectrophotometry, Asteroids, Narrowband, Spectral Reflectance, Pixels, Infrared Spectra

Scientific paper

An evaluation of CCD reflectance narrowband spectrophotometry of J VI Himalia indicates that this body is a C-class asteroid. If the theory that a parent asteroid had been captured and shattered into the four pieces now known as J VI Himalia, J VII Elara, J X Lysithea, and J XIII Leda, then by implication these other three moons of Jupiter will display a similar geological composition, as presently indicated.

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